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A Three-Dimensional Analysis of the Galactic Gamma-Ray Emission Resulting from Cosmic-Ray Interactions with the Interstellar Gas and Radiation FieldsThe primary task objective is to construct a 3-D model for the distribution of high-energy (20 MeV - 30 GeV) gamma-ray emission in the Galactic disk. Under this task the contractor will utilize data from the EGRET instrument on the Compton Gamma-Ray Observatory, H I and CO surveys, radio-continuum surveys at 408 MHz, 1420 MHz, 5 GHz, and 19 GHz, the COBE Diffuse Infrared Background Experiment (DIRBE) all-sky maps from 1 to 240 microns, and ground-based B, V, J, H, and K photometry. The respective contributions to the gamma-ray emission from cosmic ray/matter interactions, inverse Compton scattering, and extragalactic emission will be determined.
Document ID
20000059203
Acquisition Source
Goddard Space Flight Center
Document Type
Contractor or Grantee Report
Authors
Sodroski, Thomas J.
(Space Applications Corp. Largo, MD United States)
Dwek, Eli
(Space Applications Corp. Largo, MD United States)
Date Acquired
August 19, 2013
Publication Date
June 5, 2000
Subject Category
Space Radiation
Report/Patent Number
Rept-1042-006/FINAL
Funding Number(s)
CONTRACT_GRANT: NAS5-98191
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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